Coronal Magnetic Field Measurements

By Haosheng Lin, J. Kuhn, R. Coulter. 2004

281 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8f214711a08ed57e9a789cb50dbd5d9bffdc1304

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Citations in the corpus

Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “Having the ability to make direct and routine measurements of the coronal magnetic field would complement the photospheric data (Lin et al. 2004; Judge et al. 2013).”
The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, unknown): “Direct information about coronalmagnetic fields has proved elusive to date, as routine and comprehensive coronal magnetic field observations are only now beginning to become available (Lin et al. 2004; Tomczyk 2004).”
Coronal Seismology by Means of Kink Oscillation Overtones (2009, result): “On average, the magnetic field strength is expected to decrease with height above the photosphere and the results of Lin et al. (2004) seem to confirm this.”
An Instrument to Measure Coronal Emission Line Polarization (2008, methodology): “…the nearly four decades since the detection of the Zeeman effect of the coronal green line (Harvey, 1969), coronal Zeeman measurements have not been productive until recently due to advances in the technology of near-IR detector arrays (Lin, Penn, and Tomczyk, 2000; Lin, Kuhn, and Coulter, 2004).”
Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, background): “Some attempts to measure the density were undertaken (Aschwanden et al. 2003) and the average value of the magnetic field was estimated by Lin et al. (2000, 2004), but the error bars on the results are large.”
Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, methodology): “It is very difficult to make direct measurements of magnetic field strength variation in the corona, although recently there has been some progress made using spectropolarimetry by Article published by EDP Sciences Lin et al. (2004).”
Preprocessing of Vector Magnetograph Data for a Nonlinear Force-Free Magnetic Field Reconstruction (2006, background): “…extrapolations, vector magnetogram, SFT Abbreviations: KAP – Kluwer Academic Publishers; compuscript – Electronically submitted article JEL codes: D24, L60, 047 Nomenclature: KAP – Kluwer Academic Publishers; compuscript – Electronically submitted article Solar Physics, Vol. 233, 215-232 (2006)”